Solar Terrestrial Activity Report

Activity chart

Last major update issued on April 17, 2016 at 04:15 UT.

Charts (* = updated daily) Data and archive
  Solar wind (*) Solar and geomagnetic data - last month (*)
  Electron fluence (*) Archived daily reports and monthly data from 2003.01 (April 2, 2016)
Solar cycle Solar cycles 23-24 (April 2, 2016) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24 progress (April 2, 2016) Noon SDO sunspot count 1K / 4K (*)
  Solar cycles 1-24 (July 17, 2015) POES auroral activity level October 2009 - December 2012
  Comparison of cycles 21, 22, 23 and 24 (April 2, 2016) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12, 13, 14, 16 and 24 (April 2, 2016) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (March 12, 2016)  

Recent activity

The geomagnetic field was quiet to unsettled on April 16. Solar wind speed at SOHO ranged between 346 and 465 km/s. A weak disturbance, source unknown, arrived at ACE near 05 UT.

Solar flux at 17h UTC on 2.8 GHz was 109.5 (increasing 21.9 over the last solar rotation, the measurement at 20h UT was enhanced by a C5 flare in AR 12529). The 90 day 10.7 flux at 1 AU was 97.1. The Potsdam WDC planetary A index was 10 (STAR Ap - based on the mean of three hour interval ap indices: 9.6). Three hour interval K indices: 11222333 (planetary), 00342423 (Boulder).

The background x-ray flux is at the class B3 level.

At the time of counting spots (see image time), spots were observed in 4 active regions using 2K resolution (SN: 81) and 4 active regions using 1K resolution (SN: 58) SDO images on the visible solar disk.

Region 12529 [N10W40] decayed slightly in the intermediate spot section. An M class flare is still possible.
Region 12531 [N14E25] reemerged with tiny spots.
New region 12532 [N07E68] rotated into view on April 15 and was numbered the next day by SWPC.

Spotted regions not numbered (or interpreted differently) by SWPC:
New region S5242 [S19E40] was observed with a tiny spot.

C2+ flares:

Magnitude Peak time (UT) Location AR Recorded by Comment
C5.8 19:58   12529 GOES15  

Flare activity (SDO/EVE/ESP XRS-B proxy)

Coronal mass ejections (CMEs)

April 14-16: No obviously Earth directed CMEs were observed in available LASCO imagery.

Coronal holes

[Coronal hole history (since October 2002)]
[Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago]

A recurrent northern hemisphere coronal hole (CH728) rotated across the central meridian on April 15-16. A recurrent trans equatorial extension of a northern hemisphere coronal hole will likely rotate into an Earth facing position on April 20-21.

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor to fair.

Forecast

The geomagnetic field is expected to be quiet to unsettled on April 17 while April 18-19 could see quiet to active conditions as CH728 becomes geoeffective.

Coronal holes (1) Coronal mass ejection (2) M and X class flares (3)
     

1) Effects from a coronal hole could reach Earth within the next 5 days. When the high speed stream has arrived the color changes to green.
2) Effects from a CME are likely to be observed at Earth within 96 hours.
3) There is a possibility of either M or X class flares within the next 48 hours.

Green: 0-30% probability, Yellow: 30-70% probability, Red: 70-100% probability.

Active solar regions


(Click on image for 2K resolution). 4K resolution. Compare to the previous day's image.
0.5K image

When available the active region map has a coronal hole polarity overlay where red (pink) is negative and blue is positive.

Data for all numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC. Comments are my own, as is the STAR spot count (spots observed at or inside a few hours before midnight) and data for regions not numbered by SWPC or where SWPC has observed no spots. SWPC active region numbers in the table below and in the active region map above are the historic SWPC/USAF numbers.

Active region Date numbered
detected
Spot count Location at midnight Area Classification SDO / HMI 4K continuum
image with magnetic polarity overlays
Comment
SWPC Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
12529 2016.04.07 18 30 11 N10W37 0720 EKI EKI beta-gamma

area: 0810

location: N10W40

12530 2016.04.10
2016.04.11
1     N08W80 0010 AXX       AR 12530 has been spotless the last two days and had the location N13W67 for the previous spot report. While it is difficult to know what SWPC has observed in this case, it is possible they observed the spot of AR S5239 (N05W93) as it was rotating out of view and assigned it incorrectly to AR 12530 with a bogus location
S5231 2016.04.11       S15W48            
12531 2016.04.12
2016.04.13
  5 2 N13E20 0010   BXO   location: N14E25
S5234 2016.04.13       S03E06          
S5236 2016.04.13       N03W38            
S5237 2016.04.14       N10E42            
S5238 2016.04.14       N24W54            
12532 2016.04.15
2016.04.16
2 5 4 N07E62 0020 CAO CAO area: 0040

location: N07E68

S5241 2016.04.15       S13W20          
S5242 2016.04.16   1 1 S19E40 0003   AXX    
Total spot count: 21 41 18  
Sunspot number: 51 81 58  (total spot count + 10 * number of spotted regions)
Weighted SN: 36 56 33  (Sum of total spot count + classification weighting for each AR. Classification weighting: X=0, R=3, A/S=5, H/K=10)
Relative sunspot number (Wolf number): 56 36 46 k * (sunspot number)
As of February 19, 2016: k = 1.1 for SWPC, k = 0.45 for MSN 2K, k = 0.80 for MSN 1K (MSN=Magnetic Sunspot Number)

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO) (4)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2014.02 170.3
(cycle peak)
166.3 146.1 (cycle peak) 110.5 (+1.2) 10.70
2014.04 143.9 144.8 112.5 116.4 (+2.1) (solar max) 7.88
2015.02 129.1 126.0 66.7 86.1 (-3.2) 9.92
2015.03 125.9 124.6 54.5 82.2 (-3.9) 16.14
2015.04 128.8 129.7 75.3 78.9 (-3.3) 10.73
2015.05 120.0 122.6 88.8 76.1 (-2.8) 8.29
2015.06 122.3 126.1 66.5 72.1 (-4.0) 13.15
2015.07 107.0 110.8 66.4 68.3 (-3.8) 8.83
2015.08 105.4 108.0 64.6 66.4 (-1.9) 14.58
2015.09 101.7 102.7 78.1 66.0 (-0.4) 15.78
2015.10 104.1 103.3 61.7 (64.6 projected, -1.4) 14.02
2015.11 109.3 106.9 63.2 (61.9 projected, -2.7) 12.09
2015.12 113.1 109.5 57.7 (59.9 projected, -2.0) 14.29
2016.01 103.4 100.1 56.6 (58.2 projected, -1.7) 9.4
2016.02 103.6 101.0 57.2 (55.9 projected, -2.3) 9.9
2016.03 91.5 90.6 54.9 (52.9 projected, -3.0) 10.58
2016.04 (97.7)   17.1 (2A) / 32.0 (2B) / 33.7 (2C) (50.2 projected, -2.7) (9.6)

1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz.
2A) Current impact on the monthly sunspot number based on the Boulder (NOAA/SWPC) sunspot number (accumulated daily sunspots / month days).
2B) Boulder SN current month average to date.
2C) STAR SDO 1K Wolf number 30 day average.
3) Running average based on the quicklook and definitive Potsdam WDC ap indices. Values in red are based on the definitive international GFZ Potsdam WDC ap indices.
4) Updated to new data set from WDC-SILSO on July 1, 2015

This report has been prepared by Jan Alvestad. It is based on the analysis of data from whatever sources are available at the time the report is prepared. All time references are to Universal Time. Comments and suggestions are always welcome.

SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.